Results 231 to 240 of about 12,207 (244)
False positives in gravitational wave campaigns: the electromagnetic perspective. [PDF]
Oates S.
europepmc +1 more source
Proton first: rationalizing a proton transfer in a protein‐fragment complex
We present a combination of experimental and theoretical approaches to decipher the molecular recognition event of benzoic acid complexed with Protein Kinase A. The publicly known crystal structure suggests the protonated form of benzoic acid to be complexed with Protein Kinase A.
Helge Vatheuer+6 more
wiley +1 more source
Stellar structure via truncated M-fractional Lane-Emden solutions. [PDF]
Nouh MI+5 more
europepmc +1 more source
Magnetar emergence in a peculiar gamma-ray burst from a compact star merger. [PDF]
Sun H+44 more
europepmc +1 more source
A connection between proto-neutron-star Tayler-Spruit dynamos and low-field magnetars. [PDF]
Igoshev A+5 more
europepmc +1 more source
When superfluidity meets superconductivity in the extraction of <sup>3</sup>He isotope from liquid helium. [PDF]
Kempiński W+7 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Physical Review Letters, 1993
We calculate properties of neutron star matter at subnuclear densities using an improved nuclear Hamiltonian. Nuclei disappear and the matter becomes uniform at a density of about 0.6n(s), where n(s) of about 0.16/cu fm is the saturation density of nuclear matter. As a consequence, the mass of matter in the crusts of neutron stars is only about half as
D. G. Ravenhall+2 more
openaire +3 more sources
We calculate properties of neutron star matter at subnuclear densities using an improved nuclear Hamiltonian. Nuclei disappear and the matter becomes uniform at a density of about 0.6n(s), where n(s) of about 0.16/cu fm is the saturation density of nuclear matter. As a consequence, the mass of matter in the crusts of neutron stars is only about half as
D. G. Ravenhall+2 more
openaire +3 more sources